Table 1
Overview of the multi-wavelength observations in ELAIS-N1 used for this work.
| Telescope | Instrument | Survey | Wavelength cov | Area (deg2) | Depth |
|---|---|---|---|---|---|
| LOFAR | LoTSS Deep Fields | 150 MHz | ~25 | ~20 μJy beam−1 | |
| Herschel | SPIRE | HerMES | 250, 350, 500 μm | 7.16 | 4 mJy |
| PACS | HerMES | 110, 170 μm | 7.13 | 12.5/17.5 mJy | |
| Spitzer | MIPS | SWIRE | 24 μm | 7.16 | 20 mJy |
| IRAC | SWIRE | 3.6, 4.5, 5.8, 8.0 μm | 9.32 | ~22.2 mag | |
| SERVS | 3.6, 4.5 μm | 2.39 | 24.1 mag | ||
| UKIRT | WFCAM | UKIDSS-DXS | J and K | 8.87 | ~23.0 mag |
| Haleakala Observatory | PanSTARRS | Medium Deep Survey | grizy | 8.05 | ~24.7 mag |
| Subaru Telescope | HSC | SSP survey | grizy, NB816, NB921 | 7.70 | ~24.5 mag |
| CFHT | MegaCam | SpARCS | u | 11.81 | 25.4 mag |
Notes. The area covered by each survey and typical depths (3σ) per survey, except for SPIRE, PACS, and MIPS, are adopted from Kondapally et al. (2021); the detailed 3σ depths per filter are available in that paper. The depths for SPIRE, PACS, and MIPS are given by flux limits in mJy. Details on the optical Panoramic Survey Telescope and Rapid Response System (PanSTARRS) Medium Deep Survey, the HSC-SSP survey, and the Canada France Hawaii Telescope (CFHT) MegaCam SpARCS are available in Chambers et al. (2016), Aihara et al. (2018b), and Wilson et al. (2009), respectively. A detailed description of the UKIRT Infrared Deep Sky Survey - Deep Extragalactic Survey (UKIDSS-DXS) conducted with the Wide Field Camera (WFCAM) on the United Kingdom Infrared Telescope (UKIRT) can be found in Lawrence et al. (2007). The Herschel Multi-tiered Extragalactic Survey (HerMES) is described inOliver et al. (2012), and the Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE) and Spitzer Extragalactic Representative Volume Survey (SERVS) are described in Lonsdale et al. (2003) and Mauduit et al. (2012), respectively.
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